The Atmospheres of Venus and MarsJohn C. Brandt, Michael B. McElroy Retells five classic eerie stories in pop-up format, including "Dracula's Guest" and "The Masque of the Red Death." |
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Page 41
... errors are always largest for nearly - grazing angles , very sensitive combinations being those involving the angle ... error of 1 unit in the fifth decimal if the integration was performed with quadratic T - integration , At = 0.0025 ...
... errors are always largest for nearly - grazing angles , very sensitive combinations being those involving the angle ... error of 1 unit in the fifth decimal if the integration was performed with quadratic T - integration , At = 0.0025 ...
Page 42
... errors had gone up by a factor 100 at g = 0.75 and g = −0 · 75 . Taking 14 gauss points at these values of g restored the precision , bringing the error below 3 x 10-6 . A similar experience was obtained with values of g even closer to ...
... errors had gone up by a factor 100 at g = 0.75 and g = −0 · 75 . Taking 14 gauss points at these values of g restored the precision , bringing the error below 3 x 10-6 . A similar experience was obtained with values of g even closer to ...
Page 153
... error limits . A realistic assessment of the errors is difficult , even if one has all the evidence . Nevertheless , I feel it essential to place some kind of limits on the curve . It must be differentiated to find the scale height ...
... error limits . A realistic assessment of the errors is difficult , even if one has all the evidence . Nevertheless , I feel it essential to place some kind of limits on the curve . It must be differentiated to find the scale height ...
Contents
Preface | 1 |
Introductory Comments on Venuss Lower Atmosphere | 15 |
Multiple Light Scattering in Planetary Atmospheres | 35 |
Copyright | |
9 other sections not shown
Common terms and phrases
absorption albedo altitude angle atmos atmosphere of Mars band Belton Brandt/McElroy BRAZZA calculated Chamberlain and McElroy cloud cm³ sec-1 CO₂ coefficient computations cross-sections curve diffusion Earth effect electron density energy loss equation Eshleman estimates excitation exospheric exospheric temperature F₁ F₂ Figure Fjeldbo flux G. P. Kuiper Geophys Goody heat Hunten infrared ionization ionosphere isotropic JUIN Kitt Peak Kliore Kuiper layer loss rate lower atmosphere magnetic field magnetosheath Mariner Martian atmosphere Martian ionosphere Martian upper atmosphere measurements mesopause method N.MEXICO N₂ neutral number density observed obtained occultation optical optical depth optical thickness particles peak phase function photoelectrons planet planetary plasma scale pure CO2 radiation radiative Rasool reaction recombination refractivity region rotation scale height scattering solar wind Space Sci spectra spectrum Spinrad surface pressure thermal thermopause thermosphere thick tion vertical water vapor wave wavelength